Black Hole evaporation: A Perspective from Loop Quantum Gravity
arXiv:2001.08833 · doi:10.3390/universe6020021
Abstract
A personal perspective on the black hole evaporation process is presented using as guidelines inputs from: (i) loop quantum gravity, (ii) simplified models where concrete results have been obtained, and, (iii) semi-classical quantum general relativity. On the one hand, the final picture is conservative in that there are concrete results that support each stage of the argument, and there are no large departures from general relativity or semi-classical gravity in tame regions outside macroscopic black holes. On the other hand it argues against certain views that are commonly held in many quarters, such as: persistence of a piece of singularity that constitutes a part of the final boundary of space-time; presence of an \emph{event} horizon serving as an absolute barrier between the interior and the exterior; and the (often implicit) requirement that purification must be completed by the time the `last rays' representing the extension of this event horizon reach .
25 pages, 8 Figures. Invited article for a special issue "Probing New Physics with Black Holes", edited by Aurelien Barrau
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- Properties of the spherically symmetric polymer black holes
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- Gravitational lensing by a black hole in effective loop quantum gravity
- Improved Effective Dynamics of Loop-Quantum-Gravity Black Hole and Nariai Limit
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- Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the Galactic Center
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- Quantum dynamics of the black hole interior in LQC
- Exploring non-singular black holes in gravitational perturbations
- Trapping Horizons of the Evolving Charged Wormhole and Black Bounce
- Null Infinity as a Weakly Isolated Horizon
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- Nonexistence of quantum black and white hole horizons in an improved dynamic approach
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- Models of cosmological black holes
- Symmetric black-to-white hole solutions with a cosmological constant
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- Unitarity and the information problem in an explicit model of black hole evaporation
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- Expansion operators in spherically symmetric loop quantum gravity
- Exploring non-perturbative effects on quasi-topological black hole thermodynamics
- Semi-classical imprints on quasinormal mode spectra
- Dynamical Horizon Segments and Spacetime Isometries
- Dynamical Horizons and Black Hole Soft Hair
- Extended geometry of Gambini-Olmedo-Pullin polymer black hole and its quasinormal spectrum
- Black holes and their horizons in semiclassical and modified theories of gravity